Fig. 7.
EW of MGIIB for Mg II emitters (cyan triangles) and absorbers (magenta diamonds) as function of the stellar mass (left panel) and UV absolute magnitude at 1600 Å (right panel), color-coded accordingly to the redshift. The gray shaded area indicates the threshold values used to identify Mg II emitters (EW < −1.0) and absorbers (EW > 1.0).
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